The study of dark energy in various non GR based backgrounds have gathered a deep interest in recent times, particularly as several such theories have distinct features which are not present in the usual dark energy regimes based in GR. These cosmological backgrounds are very diversely motivated themselves and have their origins in various. For example,a lot of works have considered the possibility of viable scalar field based dark energy regimes in quantum gravity corrected cosmologies like the RS-II Braneworld and Loop Quantum Cosmology [1]}, [2]}, [3]}, [4]}, [5]}. There has been substantial work on new dark energy models based on thermodynamic modifications like modified area-entropy relations as well[6]}, [7]}, [8]}, [9]}, [10]}, [11]}. A great amount of literature has also been devoted to look out for exotic dark energy regimes based in cosmologies where the generalized uncertainty principles [12]}, [13]}, [14]} are considered instead of the usual Heisenberg uncertainty criterion [15]}, [16]}, [17]}. There has been a lot of work devoted towards studying dark energy regimes in non-canonical approaches like DBI etc. as well [18]}, [19]}, [20]}, [21]}, [22]}, [23]}, [24]}.
